锆石U-Pb-Hf同位素对印度南部东达尔瓦克拉通东北部新元古代花岗岩岩石成岩过程的制约作用

IF 2.9 2区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS Lithos Pub Date : 2024-09-14 DOI:10.1016/j.lithos.2024.107807
B. Vikram Raju , Ajay Dev Asokan , Xiao-Ping Xia , Zexian Cui , Arathi G. Panicker , M. Ram Mohan
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引用次数: 0

摘要

在本研究中,我们整合了来自东达尔沃克拉通(EDC)东北部的高K新元古代花岗岩的大块岩石化学和原位锆石U-Pb-Hf同位素,研究了它们的来源、成岩过程和可能的构造环境。根据矿物组合及其地球化学特征,这些花岗岩被划分为角闪石-黑云母花岗岩(HBG)与微晶飞地(ME)、黑云母花岗岩(BTG)和蒙祖花岗岩(MG)。野外观测和锆石U-Pb年龄显示,这些花岗岩是在2.53至2.50 Ga之间同时形成的。HBG(包括ME)具有低二氧化硅、金属铝亲和性和高铁镁元素含量,这与它们源自黑云母来源是一致的。一些 HBG 和 ME 样品的不相容元素含量很高,与沙努基多岩类似。HBG和ME的地球化学属性和强烈演化的锆石Hf同位素组成(ɛHf(t)=-4.3至+1.8和-7.3至+0.2)表明它们来源于经俯冲沉积物变质的地幔源。BTG和MG的成分相似,二氧化硅含量高,铁镁元素含量低,过铝亲和性适中,这表明它们来自长粒地壳。这些花岗岩的亚火成岩至火成岩锆石Hf同位素组成(ɛHf(t) = -2.7 至 +1.4 和 -6.9 至 +1.9 )支持异质古地壳来源的参与。虽然所有花岗岩都表现出相似的锆石 Hf 同位素组成,但它们的地球化学属性却显示出不同的来源。HBG反映了幼年地壳的补充,而BTG和MG则是地壳再加工的产物。我们认为,这些花岗岩是在向东俯冲板块断裂后西达尔瓦板块和东达尔瓦板块之间的大陆-大陆碰撞过程中形成的。板块断裂和/或加厚地壳的岩石圈分层引起的星体层上涌导致了变质地幔岩浆的形成,从而推动了地壳再加工。所观察到的 EDC 花岗岩的锆石 Hf 同位素组成与现今的新生代阿尔卑斯山-喜马拉雅山型造山运动相似,支持先俯冲后大陆碰撞的模式,从而稳定了 Archean 岩石圈。EDC这一部分存在古中新世长岩地壳的证据值得进一步研究,以检验达尔瓦克拉通的三岩模型。
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Zircon U-Pb-Hf isotopes constraints on the petrogenesis of Neoarchean granitic rocks from the Northeastern part of the Eastern Dharwar Craton, Southern India
In the present study, we integrate bulk rock chemistry and in-situ zircon U-Pb-Hf isotopes of high-K Neoarchean granitoids from the northeastern part of the Eastern Dharwar Craton (EDC) to investigate their source, petrogenesis, and plausible tectonic setting. Based on the mineral assemblage, in coherence with their geochemical characteristics, these granitoids are classified as Hornblende-biotite granite (HBG) with Microgranular enclaves (ME), Biotite granite (BTG) and Monzogranite (MG). Field observations and zircon U-Pb ages reveal coeval emplacement of these granitoids between 2.53 and 2.50 Ga. The HBG, including ME, has low silica, metaluminous affinity, and high ferromagnesian element content, consistent with their derivation from a mafic source. Some of the HBG and ME samples are strongly enriched in incompatible elements, similar to the sanukitoids. The geochemical attributes and strongly evolved zircon Hf isotopic compositions (ɛHf(t) = −4.3 to +1.8 and −7.3 to +0.2) of the HBG and ME suggest their derivation from a mantle source metasomatized by subducted sediments. The BTG and MG are compositionally similar, with high silica, low ferromagnesian element content, and moderate peraluminous affinity, suggesting the involvement of felsic crustal sources. The sub-chondritic to chondritic zircon Hf isotopic compositions (ɛHf(t) = −2.7 to +1.4 and  −6.9 to +1.9) of these granitoids support the involvement of heterogeneous ancient crustal sources. While all granitoids exhibit similar zircon Hf isotopic compositions, their geochemical attributes suggest distinct sources. The HBG reflects juvenile crustal additions, whereas BTG and MG are products of the crustal reworking. We propose that these granitoids formed during the continent-continent collision between Western and Eastern Dharwar cratons, that took place after the break-off of the eastward subducting slab. The asthenospheric upwelling induced by slab break-off and/or lithospheric delamination of thickened crust led to the genesis of metasomatized mantle derived magma, which drove the crustal reworking. The observed zircon Hf isotopic composition of the EDC granitoids are similar to the present day Phanerozoic Alpine-Himalayan type orogenies supporting subduction followed by continental collision model for the stabilisation of Archean cratons. Evidence for the existence of Paleo- Mesoarchean felsic crust from this part of the EDC warrants further studies to test the three-terrane model for the Dharwar Craton.
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来源期刊
Lithos
Lithos 地学-地球化学与地球物理
CiteScore
6.80
自引率
11.40%
发文量
286
审稿时长
3.5 months
期刊介绍: Lithos publishes original research papers on the petrology, geochemistry and petrogenesis of igneous and metamorphic rocks. Papers on mineralogy/mineral physics related to petrology and petrogenetic problems are also welcomed.
期刊最新文献
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